Revisiting Isocurvature Bounds on the Minimal QCD Axion

TL;DR

This paper revisits the isocurvature bounds on the minimal QCD axion, showing that these constraints can be evaded under certain UV physics conditions, especially with a small quartic coupling affecting $f_a$ during inflation.

Contribution

It demonstrates that isocurvature bounds on the QCD axion are not absolute and can be avoided when the PQ-breaking field's quartic coupling is small, altering $f_a$ during inflation.

Findings

Isocurvature bounds depend on UV physics and can be evaded.

Small quartic coupling suppresses isocurvature perturbations.

Large regions of parameter space remain viable for high $f_a$ and $H_I$.

Abstract

The QCD axion has important connections to early universe cosmology. For example, it is often said that isocurvature limits rule out a combination of high axion decay constant, $f_a$, and high inflationary Hubble scale, $H_I$. High scales are theoretically motivated, so it is important to ask how robust this constraint is. We demonstrate that this constraint is naturally evaded when the quartic coupling of the complex $U(1)_\mathrm{PQ}$-breaking field is small. In this case, $f_a$ changes from a larger value during inflation to a smaller value in the later universe, suppressing isocurvature perturbations. Importantly, we show that in large parts of parameter space this solution is not jeopardised by overproduction of the axion through parametric resonance. The isocurvature bounds are thus dependent on UV physics. We have found that, even for the minimal QCD axion, large parts of UV parameter space at both high $f_a$ and high $H_I$ are in fact allowed, not ruled out by isocurvature constraints.